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Related papers: NGC 4244: A Low Mass Galaxy with a Falling Rotatio…

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In a previous paper (Olling 1995, \aj, 110, 591; astro-ph/9505002) a method was developed to determine the shapes of dark matter halos of spiral galaxies from an accurate determination of the rotation curve, the flaring of the gas layer and…

Astrophysics · Physics 2009-10-28 Rob P. Olling

In a previous paper (Olling 1995, astro-ph/9505002) a method was developed to determine the shapes of dark matter halos of spiral galaxies from an accurate determination of the rotation curve, the flaring of the gas layer and the velocity…

Astrophysics · Physics 2007-05-23 Rob P. Olling

In a previous paper (Paper I) a method was developed to determine the shapes of dark matter halos of spiral galaxies from the flaring and velocity dispersion of the gas layer. Here I present the results for the almost edge-on Scd galaxy NGC…

Astrophysics · Physics 2007-05-23 Rob P. Olling

We present 21-cm observations and models of the HI kinematics and distribution of NGC 4244, a nearby edge-on Scd galaxy observed as part of the Westerbork Hydrogen Accretion in LOcal GAlaxieS (HALOGAS) survey. Our models give insight into…

Astrophysics of Galaxies · Physics 2011-07-21 Laura K. Zschaechner , Richard J. Rand , George H. Heald , Gianfranco Gentile , Peter Kamphuis

We have obtained deep surface photometry of the edge-on spiral galaxy NGC 4244. Our data reliably reach 27.5 R magnitude arcsec^{-2}, a significant improvement on our earlier deep CCD surface photometry of other galaxies. NGC 4244 is a…

Astrophysics · Physics 2016-08-30 Anne M. Fry , Heather L. Morrison , Paul Harding , Todd A. Boroson

We study the vertical gradient in azimuthal velocity of spiral galaxy NGC 4244 in a thin disk model. With surface density accounting for the rotation curve, we model the gradient properties in the approximation of quasi-circular orbits and…

Astrophysics of Galaxies · Physics 2015-07-02 Joanna Jałocha , Łukasz Bratek , Szymon Sikora , Marek Kutschera

We present new HI observations of the nearby dwarf galaxy NGC 3741. This galaxy has an extremely extended HI disk, which allows us to trace the rotation curve out to unprecedented distances in terms of the optical disk: we reach 42 B-band…

Astrophysics · Physics 2008-11-26 G. Gentile , P. Salucci , U. Klein , G. L. Granato

We present a study of the HI distribution and dynamics of the nearby spiral galaxy NGC5055 based on observations with the Westerbork Synthesis Radio Telescope. The gaseous disk of NGC5055 extends out to about 40 kpc, equal to 3.5 R_25, and…

Astrophysics · Physics 2009-11-11 G. Battaglia , F. Fraternali , T. Oosterloo , R. Sancisi

NGC 4013 is a distinctly warped galaxy with evidence of disk-halo activity. Through deep HI observations and modeling we confirm that the HI disk is thin (central exponential scale height of with an upper limit of 4" or 280 pc), but…

Astrophysics of Galaxies · Physics 2015-08-06 Laura K. Zschaechner , Richard J. Rand

The thickness of the neutral hydrogen layer, coupled with the rotation curve, traces the outer dark matter potential. We estimate the amplitude of the flaring in spiral galaxies from a 3D model of the HI gas. Warps in particular are…

Astrophysics · Physics 2007-05-23 J. -F. Becquaert , F. Combes

We present spectroscopic observations of the stellar motions in the disk of the superthin edge-on spiral galaxy IC 5249 and re-analyse synthesis observations of the HI. We find that the HI rotation curve rises initially to about 90-100…

Astrophysics · Physics 2009-11-07 P. C. van der Kruit , J. Jimenez-Vicente , M. Kregel , K. C. Freeman

Neutral hydrogen observations of the nearby, edge-on spiral galaxy NGC 891 reveal the presence of an HI halo extending up to at least 5 kpc from the plane. This halo gas appears to rotate 25 to 100 km/s more slowly than the gas in the…

Astrophysics · Physics 2009-05-29 R. A. Swaters , R. Sancisi , J. M. van der Hulst

We present the preliminary detection of a stellar halo in the nearby, edge-on galaxy, NGC 4244. Using data from the Hubble Space Telescope's Advanced Camera for Surveys (HST/ACS), we have examined number counts of red giant branch (RGB)…

Astrophysics · Physics 2009-11-13 Anil Seth , Roelof De Jong , Julianne Dalcanton , the GHOSTS team

We present observations of the nuclear star cluster in the nearby edge-on spiral galaxy NGC 4244 using the Gemini Near-Infrared Integral Field Spectrograph (NIFS) with laser guide star adaptive optics. From a previous study of edge-on…

We present deep, high velocity resolution (~1.6 km/s) Giant Meterwave Radio Telescope (GMRT) HI 21cm synthesis images of the faint (M_B ~ -10.6) local group dwarf galaxy DDO210. We find that the HI distribution in the galaxy is not…

Astrophysics · Physics 2009-11-10 Ayesha Begum , Jayaram N. Chengalur

The edge-on galaxy NGC 4565 has been observed in the 12CO(J=1-0)-line emission using the Nobeyama 45-m telescope with an angular resolution of 15". We obtained a scan along the major axis for +/-5' (+/- 15 kpc) about the galactic center,…

Astrophysics · Physics 2007-05-23 Y. Sofue , N. Nakai

We present new HI spectral line images of the nearby low-mass galaxy NGC 5238, acquired with the Karl G. Jansky Very Large Array (VLA). Located at a distance of 4.51+/-0.04 Mpc, NGC 5238 is an actively star-forming galaxy with widespread…

We present observations of the distribution and kinematics of neutral and ionized gas in NGC 1144, a galaxy that forms part of the Arp 118 system. Ionized gas is present over a huge spread in velocity (1100 km/s) in the disk of NGC 1144,…

Astrophysics · Physics 2009-10-31 M. A. Bransford , P. N. Appleton , C. F. McCain , K. C. Freeman

We have analyzed high velocity resolution HI synthesis observations of the nearly face-on Sc galaxy NGC 1232. The neutral gas distribution extends well beyond the optical extent of the galaxy. As expected, local peaks in the HI column…

Astrophysics · Physics 2009-10-31 L. van Zee , J. Bryant

We present UBVJHKHalpha and HI data of the irregular galaxy NGC 2366. It is a normal boxy-shaped disk seen at high inclination angle. We do not see any unambiguous observational signature of a bar. There is an asymmetrical extension of…

Astrophysics · Physics 2009-11-06 D. A. Hunter , B. G. Elmegreen , H. van Woerden
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